Can a White Dwarf Collapse into a Neutron Star Without a Supernova?

In summary: The collapse of a neutron star beyond its Tolman-Oppenheimer-volkoff limit would always result in the formation of a black hole. There is no possibility of fusion reactions occurring in a neutron star, as it is already formed of the fusion of its neutrons.
  • #1
PeterB
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Is it possible for white dwarf star in binary system where it is feeding off its partner star to collapse directly into a neutron star? Or is something inherent in the formation of neutron stars where they must be formed from supernova?
 
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  • #2
When a white dwarf accretes mass from a companion and exceeds the Chandrasekhar limit of about 1.4 solar masses, instead of collapsing to a neutron star, it explodes as a Type 1A supernova. The reason is that a white dwarf is formed of relatively light elements like carbon and oxygen, so there is still a lot of thermonuclear energy available from further fusion reactions. So when the star gets compressed further, these thermonuclear reactions ignite and the star explodes in a massive explosion. By contrast, when the core of a more massive star collapses to form a neutron star, the core is formed of heavier elements like iron. Since iron is at the peak of the nuclear binding energy curve, there is no more thermonuclear energy available from further fusion reactions.
 
  • #3
Thank you for you response, Would this mean that a neutron star which exceeds its Tolman-Oppenheimer-volkoff limit would always collapse to a black hole? Would fusion of Neutron star material (primarily neutrons) be possible?
 
  • #4
Big neutron star collapse results in a black hole. The core of a neutron star can be thought of as the "fusion" of its neutrons. However there is no such thing as a fusion reaction in this case.
 
  • #5
PeterB said:
Thank you for you response, Would this mean that a neutron star which exceeds its Tolman-Oppenheimer-volkoff limit would always collapse to a black hole?

Yes, as far as we know this is the only outcome.
 

1. How does a white dwarf become a neutron star?

A white dwarf becomes a neutron star through a process called electron capture. As the white dwarf's core reaches a critical density, the electrons are forced to combine with protons to form neutrons. This process releases a large amount of energy and causes the white dwarf to collapse into a neutron star.

2. What is the main difference between a white dwarf and a neutron star?

The main difference between a white dwarf and a neutron star is their composition. A white dwarf is made up of highly compressed degenerate matter, while a neutron star is made up of even denser neutron-rich matter. Additionally, a white dwarf is supported by electron degeneracy pressure, while a neutron star is supported by neutron degeneracy pressure.

3. How long does it take for a white dwarf to become a neutron star?

The process of a white dwarf becoming a neutron star can take millions of years. It depends on the mass of the white dwarf and the rate at which it is accreting matter from a companion star. Once the critical density is reached, the collapse into a neutron star can happen very quickly, within a matter of seconds.

4. Can a white dwarf skip the neutron star stage and become a black hole?

No, a white dwarf does not have enough mass to directly collapse into a black hole. The Chandrasekhar limit, which is the maximum mass a white dwarf can have before collapsing into a neutron star, is about 1.4 times the mass of the sun. To become a black hole, a star needs to have a mass at least three times greater than the sun's mass.

5. How are neutron stars detected?

Neutron stars can be detected through their emission of electromagnetic radiation, such as radio waves, X-rays, and gamma rays. They can also be detected through their effects on nearby matter, such as creating accretion disks in binary systems. In some cases, neutron stars can also be detected through gravitational waves, which are ripples in space-time caused by the star's extreme gravitational pull.

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